Spectral analysis and model atmospheres of WR type central stars
Wolf-Rayet type spectra of central stars are compared with spectra from Pop. I objects. Non-LTE models for expanding atmospheres are applied for analyzing these spectra quantitatively.
In: Astrophysics and Space Science: 1996 , 238, 31
Proceedings of the workshop on "Planetary Nebulas with WR Type Nuclei", Island Ven, Sweden, August 1995 (in press)
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